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The results include the observations of various electromagnetic and electrostatic wave modes in the induced magnetosphere of Venus: strong emissions of ∼100 Hz whistler waves are observed in addition to electrostatic ion acoustic waves, solitary structures and Langmuir waves in the magnetosheath of Venus. We used the data products provided by the different subsystems of RPW to study Venus’ induced magnetosphere. They include the identification of a number of magnetospheric plasma wave modes, measurements of the electron number densities computed using the quasi-thermal noise spectroscopy technique and inferred from the probe-to-spacecraft potential, the observation of dust impact signatures, kinetic solitary structures, and localized structures at the bow shock, in addition to the validation of the wave normal analysis on-board from the Low Frequency Receiver. In this paper, we review the main observations of the RPW instrument during VGAM1. While this flyby was performed to provide the spacecraft with sufficient velocity to get closer to the Sun and observe its poles from progressively higher inclinations, the Radio and Plasma Wave (RPW) consortium, along with other operational in situ instruments, had the opportunity to perform high cadence measurements and study the plasma properties in the induced magnetosphere of Venus.Īims. On December 27, 2020, Solar Orbiter completed its first gravity assist manoeuvre of Venus (VGAM1). Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USAĮuropean Space Agency (ESA), European Space Astronomy Centre (ESAC), Camino Bajo del Castillo s/n, 28692 Villanueva de la Cañada, Madrid, SpainĬontext. Institute of Atmospheric Physics of the Czech Academy of Sciences, Prague, Czech Republic 35, 01187 Dresden, GermanyĪstronomical Institute of the Czech Academy of Sciences, Prague, Czech Republic Technische Universität Dresden, Wärzburger Str. Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USAĭepartment of Space and Plasma Physics, School of Electrical Engineering and Computer, Stockholm, SwedenĬNES, 18 Avenue Edouard Belin, 31400 Toulouse, France Physics Department, University of California, Berkeley, CA, USAĭepartment of Physics, Imperial College, SW7 2AZ London, UK School of Physics and Astronomy, University of Glasgow, G12 8QQ Glasgow, UKĭepartment of Physics and Astronomy, University of Iowa, Iowa City, IA 52242-1479, USA
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Pavlou str., Pedeli, 15236 Athens, Greece National Observatory of Athens, IAASARS, Metaxa and Vas. Space and Plasma Physics, KTH Royal Institute of Technology, 10405 Stockholm, Swedenįaculty of Mathematics and Physics, Charles University, Prague, Czech Republicĭepartment of Astrophysics, Astronomy and Mechanics, Faculty of Physics, School of Science National and Kapodistrian University of Athens, 15783 Zographos, Greeceĭepartment of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI, USA Istituto per la Scienza e Tecnologia dei Plasmi (ISTP), Consiglio Nazionale delle Ricerche, Via Amendola 122/D, 70126 Bari, Italy Space Sciences Laboratory, University of California, Berkeley, CA, USA Space Research Institute, Austrian Academy of Sciences, Graz, Austria Johns Hopkins Applied Physics Lab, Laurel, MD 20723, USA Radboud Radio Lab, Department of Astrophysics, Radboud University, Nijmegen, The Netherlands LPC2E, CNRS, University of Orléans, 3A avenue de la recherche scientifique, Orléans, France LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France LPP, CNRS, Observatoire de Paris, PSL Research University, Sorbonne Université, École Polytechnique, Institut Polytechnique de Paris, 91120 Palaiseau, FranceĮ-mail: Institute of Space Physics, Box 537 75121 Uppsala, Swedenĭepartment of Space Physics, Institute of Atmospheric Physics of the Czech Academy of Sciences, Prague, Czech Republic Astronomical objects: linking to databases.Including author names using non-Roman alphabets.
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